Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

Eric Poisson

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arXiv · gr-qc/9801038

Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

Eric Poisson

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Abstract

The accuracy of the post-Newtonian waveforms, both in standard and Pade form, is determined by computing their matched-filtering overlap integral with a reference waveform obtained from black-hole perturbation theory.

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Eric Poisson. 1998-01-12. Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms. https://arxiv.org/abs/gr-qc/9801038

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